Fraction of SFR− M_∗ bins with M_∗ > 10¹⁰ M_⊙ and with accurate dust temperature estimates (see Sect. 3.1) in our stacking analysis as function of their Δlog (SSFR)_MS (top left panel), L_IR (top right panel) or SSFR (bottom panel). Horizontal dashed lines represent the 80% completeness limits. Hatched areas represent the regions of parameter space affected by incompleteness, i.e., where less than 80% of our SFR− M_∗ bins have accurate dust temperature estimates. Shaded regions in the top left panel show the location and dispersion of the MS of star formation.